Low-Intensity States in the Neutron Star X-ray Binary Aql X-1

dc.creatorMaitra, Dipankar
dc.creatorBailyn, Charles D.
dc.date2005-10-11
dc.date.accessioned2026-07-07T06:43:49Z
dc.date.available2026-07-07T06:43:49Z
dc.descriptionAql X-1 was observed in a Low Intensity State (LIS), a state that is usually characterized by high optical but low X-ray flux. Our daily monitoring of the source using the 1.3m telescope in Cerro Tololo Inter-America Observatory operated by the Small and Moderate Aperture Research Telescope System (SMARTS) was used to trigger a series of target-of-opportunity (ToO) observations of the source using the Rossi X-ray Timing Explorer satellite (RXTE). The X-ray colors and temporal variability studies suggest that the source was in a powerlaw dominated state featuring high rms variability in the lightcurve and dominance of hard photons during this LIS. The ToO observations were continued until the source made a transition to the canonical thermal dominated or high/soft state.
dc.description5 pages, 3 figures, uses elsart.cls. Presented in "A LIFE WITH STARS" , a meeting in honor of Ed van den Heuvel, Amsterdam, 22-26 August 2005
dc.identifierhttps://arxiv.org/abs/astro-ph/0510329
dc.identifierhttp://arxiv.org/abs/astro-ph/0510329
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102563
dc.subjectAstrophysics
dc.titleLow-Intensity States in the Neutron Star X-ray Binary Aql X-1
dc.typetext

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